Results 211 to 220 of about 23,101 (234)

News feature: Seeing the ghostly universe. [PDF]

Proc Natl Acad Sci U S A, 2014
McKee M.
europepmc   +1 more source

Training and onboarding initiatives in high energy physics experiments. [PDF]

Front Big Data
Reinsvold Hall A, Skidmore N, Benelli G, Carlson B, David C, Davies J, Deconinck W, DeMuth D, Elmer P, Garg RB, Hageböck S, Lieret K, Lukashenko V, Malik S, Morris A, Schellman H, Stewart GA, Veatch J, Hernandez Villanueva M.   +18 more
europepmc   +1 more source

The <i>ν</i>-Process in the Light of an Improved Understanding of Supernova Neutrino Spectra

, 2018
André Sieverding, G. Martı́nez-Pinedo, L. Huther, K. Langanke, Alexander Heger   +4 more
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Mathematical Modeling of Physical Reality: From Numbers to Fractals, Quantum Mechanics and the Standard Model. [PDF]

Entropy (Basel)
Kupczynski M.
europepmc   +1 more source

Primordial black holes and their gravitational-wave signatures. [PDF]

Living Rev Relativ
Bagui E, Clesse S, De Luca V, Ezquiaga JM, Franciolini G, García-Bellido J, Joana C, Kumar Jain R, Kuroyanagi S, Musco I, Papanikolaou T, Raccanelli A, Renaux-Petel S, Riotto A, Ruiz Morales E, Scalisi M, Sergijenko O, Ünal C, Vennin V, Wands D, LISA Cosmology Working Group.   +20 more
europepmc   +1 more source

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SUPERNOVA NEUTRINOS

Neutrino Oscillations and Their Origin, 2002
We propose that neutrino-proton elastic scattering, {nu} + p {yields} {nu} + p, can be used for the detection of supernova neutrinos. Though the proton recoil kinetic energy spectrum is soft, with T{sub p} {approx_equal} 2E{sub {nu}}{sup 2}/M{sub p}, and the scintillation light output from slow, heavily ionizing protons is quenched, the yield above a ...
openaire   +1 more source

Neutrinos and Supernovae

AIP Conference Proceedings, 2008
Core‐collapse supernovae are one of the few astrophysical environments in which neutrinos play a dominant role. Neutrinos emission is the means by which a newly‐born neutron star formed in a core‐collapse event cools. Neutrinos may play a significant role in causing the supernova explosion. Finally neutrinos may significantly affect the nucleosynthesis
Bradley S. Meyer, P. Demetriou, R. Julin, S. V. Harissopulos   +3 more
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Neutrino Heating in Supernovae

Physical Review Letters, 1988
I argue that standard descriptions of stellar collapse omit the primary mechanism for dissipative neutrino reactions in nuclear matter, nuclear excitation by neutral-current scattering. The nuclear heating rate, due to primarily to muon- and tauon-neutrino excitation of giant resonance states, is on the order of 90 MeV/nucleon sec at a radius of 100 km.
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SUPERNOVA EXPLOSIONS AND SUPERNOVA NEUTRINOS

Neutrinos in Physics and Astrophysics, 2000
We summarize the current status of core-collapse supernova theory, in particular as it relates to multi-dimensional effects and neutrino transport . Highlighted are pulsar kicks , neutrino burst signatures, many-body effects, and observed asphericities that may have a bearing on the mechanism of supernova explosions .
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NEUTRINOS FROM SUPERNOVAE

International Journal of Modern Physics D, 1994
The historic detection of neutrinos from supernova SN1987A demonstrated that they are an invaluable source of information about neutrino properties and the dynamics of gravitational stellar collapse. A number of experiments are currently being prepared for the next detection of the supernova neutrino burst.
openaire   +1 more source